A TWISTED FLUX MODEL FOR SOLAR PROMINENCES .2. FORMATION OF A DIP IN A MAGNETIC-STRUCTURE BEFORE THE FORMATION OF A SOLAR PROMINENCE

被引：0
|
作者：
DEMOULIN, P [1 ]
PRIEST, ER [1 ]
机构：
[1] UNIV ST ANDREWS, DEPT APPL MATH, ST ANDREWS KY16 9SS, SCOTLAND
来源：
ASTRONOMY & ASTROPHYSICS | 1989年 / 214卷 / 1-2期
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
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页码：360 / 368
页数：9
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